Rotating ideal magnetohydrodynamic flow in general relativity

Details Rotating ideal magnetohydrodynamic flow in general relativity Rotating ideal magnetohydrodynamic flow in general relativity

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.152..215k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 152, no. 2, Feb. 1989, p. 215-222.

Statistics

Computation

Computational Astrophysics, Magnetohydrodynamic Flow, Relativity, Rotating Fluids, Einstein Equations, Equations Of Motion, Lorentz Force, Pressure Distribution

Scientific paper

The nonrelativistic MHD description for matter appears to be essential in the study of the large-scale properties of the universe in Newton-Maxwell cosmology and in the astrophysics of galaxies, star clusters, and of stars of all types. Here, the field equations and the equations of motion for stationary, axisymmetric, rotating, and MHD flow are presented. Exact solutions are obtained for rigid rotation and for the vanishing and nonvanishing Lorentz force.

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